Joint Inversion of Normal Mode and Body Wave Data for Inner Core Anisotropy 2
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Adam Marian Dziewoński Was Spread Upon the Permanent Records of the Faculty
At a meeting of the FACULTY OF ARTS AND SCIENCES on November 7, 2017, the following tribute to the life and service of the late Adam Marian Dziewoński was spread upon the permanent records of the Faculty. ADAM MARIAN DZIEWOŃSKI BORN: November 15, 1936 DIED: March 1, 2016 Adam Marian Dziewoński was born in Lwów, Poland (now Lviv, Ukraine) and received his M.S. in 1960 from the University of Warsaw and his Doctor of Technical Sciences in 1965 from the Academy of Mines and Metallurgy in Krakow. He moved to the United States in 1965 as a research associate at the Graduate Research Center of the Southwest in Dallas and became an assistant professor at University of Texas at Dallas in 1969. Adam moved to Harvard University as an associate professor in 1972, became a full professor in 1976, and was named the Frank B. Baird, Jr., Professor of Science in 1994. He was the chair of the Department of Geological Sciences between 1982 and 1986 (Department of Earth and Planetary Sciences thereafter). He retired in 2009 but remained actively engaged in research until his death. Adam was born in a year of seismological significance, the year in which the Earth’s inner core was discovered. As if fated, Adam was involved in all subsequent major discoveries about this deepest layer of Earth. With James Freeman Gilbert, Adam provided the first direct evidence that the inner core is solid, settling the debate over its nature. He continued his work on the inner core with his colleagues at Harvard and went on to show that it is anisotropic, rotates at a slightly different rate than the mantle, and has another layer at its center. -
DOI: 10.1126/Science.285.5431.1231 , 1231 (1999); 285 Science Miaki
Normal-Mode and Free-Air Gravity Constraints on Lateral Variations in Velocity and Density of Earth's Mantle Miaki Ishii and Jeroen Tromp Science 285, 1231 (1999); DOI: 10.1126/science.285.5431.1231 This copy is for your personal, non-commercial use only. If you wish to distribute this article to others, you can order high-quality copies for your colleagues, clients, or customers by clicking here. Permission to republish or repurpose articles or portions of articles can be obtained by following the guidelines here. The following resources related to this article are available online at www.sciencemag.org (this information is current as of August 27, 2012 ): Updated information and services, including high-resolution figures, can be found in the online version of this article at: on August 27, 2012 http://www.sciencemag.org/content/285/5431/1231.full.html This article cites 23 articles, 1 of which can be accessed free: http://www.sciencemag.org/content/285/5431/1231.full.html#ref-list-1 This article has been cited by 155 article(s) on the ISI Web of Science This article has been cited by 13 articles hosted by HighWire Press; see: http://www.sciencemag.org/content/285/5431/1231.full.html#related-urls www.sciencemag.org This article appears in the following subject collections: Geochemistry, Geophysics http://www.sciencemag.org/cgi/collection/geochem_phys Downloaded from Science (print ISSN 0036-8075; online ISSN 1095-9203) is published weekly, except the last week in December, by the American Association for the Advancement of Science, 1200 New York Avenue NW, Washington, DC 20005. -
Normal-Mode and Free-Air Gravity Constraints on Lateral Variations In
R ESEARCH A RTICLES ficient quality. There are density models based on current and past plate motions in which the Normal-Mode and Free-Air sources of heterogeneity are cold subducted slabs (5), and an upper mantle density model, Gravity Constraints on Lateral containing strong high-degree components, has been determined with surface wave data (6). Variations in Velocity and A density model of the mantle is im- portant to geophysics because mantle-flow calculations cannot be performed without Density of Earth’s Mantle it (7, 8). However, a whole-mantle den- Miaki Ishii* and Jeroen Tromp sity model is usually obtained by scaling an S velocity model, which is justifiable With the use of a large collection of free-oscillation data and additional con- if the heterogeneity has a single cause straints imposed by the free-air gravity anomaly, lateral variations in shear that affects both, for example, variations in velocity, compressional velocity, and density within the mantle; dynamic to- temperature. pography on the free surface; and topography on the 660-km discontinuity and In recent years, mainly as a result of the 9 the core-mantle boundary were determined. The velocity models are consistent June 1994 Bolivia earthquake, the quantity and with existing models based on travel-time and waveform inversions. In the quality of normal-mode, or free-oscillation, lowermost mantle, near the core-mantle boundary, denser than average ma- data have improved substantially (9), allowing terial is found beneath regions of upwellings centered on the Pacific Ocean and us to constrain the long-wavelength structure of Africa that are characterized by slow shear velocities. -
For Immediate Release Contact: Nan Broadbent 408-431-9885
For Immediate Release Contact: Nan Broadbent 408-431-9885, [email protected] Miaki Ishii honored with Richter Early Career Award Harvard professor recognized by Seismological Society of America SAN FRANCISCO -- Since her first forays into studying earthquakes, Miaki Ishii has successfully tackled seismological problems that would likely intimidate even the most seasoned researchers. In her young career, Ishii, an assistant professor of earth and planetary science at Harvard University, has made two groundbreaking discoveries in geophysics that have fostered intense debate and subsequent research that has changed the understanding of deep Earth seismology. For her work, the Seismological Society of America (SSA) will honor the 33-year-old Ishii with its Charles F. Richter Early Career Award, which honors outstanding contributions to the goals of the Society by a member early in her or his career. She will receive the award at a special ceremony at the SSA annual meeting on April 8 in Monterey, CA. Since she entered Harvard to begin her doctoral work in the late 1990s, Ishii has shown a knack for answering big questions. Shortly after her arrival at Harvard, she researched the driving force behind plate tectonics -- lateral variations in mantle density. The research inferred that the slowest parts of the lowermost mantle are denser than average, rather than lighter as most had assumed. The findings flew in the face of the long-held theory of a homogenized mantle and generated significant subsequent research and debate. Recent research is beginning to confirm Ishii’s observations. Her second groundbreaking find built on her previous study with Harvard’s Adam Dziewonski. -
15 March 2016 Magazine
VOL. 97 NO. 6 15 MAR 2016 WHERE CURIOSITY HAS TAKEN US Building Better Climate Models No Tolerance for Sexual Harassment Cheers, Yawns for Planet Nine Have an Idea or Topic to Present at the Fall Meeting? Submit a Session Proposal Deadline: 20 April, 11:59 P.M. EDT You must be current in your 2016 membership dues in order to propose a session. fallmeeting.agu.org Earth & Space Science News Contents 15 MARCH 2016 PROJECT UPDATE VOLUME 97, ISSUE 6 22 Better Tools to Build Better Climate Models A Department of Energy collaboration aims to make climate model development faster and more efficient by creating a prototype of a system for testing model components. OPINION 9 Steps to Building a No-Tolerance Culture for Sexual Harassment AGU can lead the way in building an environment where sexual and other types of harassment have no place. 16 AGU NEWS COVER 2017 Fall Meeting 26 to Go to New Orleans, 2018 to Washington, D. C. Where Curiosity Has Taken Us AGU opts to relocate its 26,000-plus- attendee meeting from San Francisco for The Curiosity rover, one of NASA’s flagship missions, analyzes 2 years to avoid detrimental impacts from Martian geology, geochemistry, climatology, and radiation to assess extensive construction at the convention whether Mars could have supported microbial life. center. Earth & Space Science News Eos.org // 1 Contents DEPARTMENTS Editor in Chief Barbara T. Richman: AGU, Washington, D. C., USA; eos_ [email protected] Editors Christina M. S. Cohen Wendy S. Gordon Carol A. Stein California Institute Ecologia Consulting, Department of Earth and of Technology, Pasadena, Austin, Texas, USA; Environmental Sciences, Calif., USA; wendy@ecologiaconsulting University of Illinois at cohen@srl .caltech.edu .com Chicago, Chicago, Ill., USA; [email protected] José D. -
SPRING 2016 TIMES Earthharvard UNIVERSITY DEPARTMENT&Planetary of EARTH and PLANETARY SCIENCES
SPRING 2016 TIMES EarthHARVARD UNIVERSITY DEPARTMENT&Planetary OF EARTH AND PLANETARY SCIENCES R/V Knorr at sunset in the Atlantic. This vessel was used during a recent five-week MARPEX cruise to collect samples from the Mid-Atlantic Ridge. Earthquakes, movies, sailing: Freshman Seminars not CEDRIC HAMELIN typical Harvard fare 4 Exploring Earth’s Final Frontier What mid-ocean ridges reveal about tectonics and magmatism BY JOCELYN FUENTES, THIRD-YEAR GRADUATE STUDENT Three siblings reflect on hen most people think of the ocean, tonic boundaries, ocean ridges are an essential part 13family traditions—and EPS they imagine a vast expanse of calm of the Earth system where the seafloor is constantly blue water with little thought for what being created through magmatism and faulting. liesW below, or they think of the water that fills the Since the first map of the ocean floor was cre- ocean basins. For many ocean scientists, however, ated, in 1977 by Marie Tharp and Bruce Heezen, what is most interesting lies beneath the water on many advances have been made in the field of the seafloor. Two-thirds of the geology of the marine geology and geophysics. In particular, our planet is there, obscured by the water above. The ability to map and image the seafloor has improved Rock Hard Bodies play most prominent feature of the seafloor is the greatly. Unfortunately, these techniques generally Meanhouse Effect in first mid-ocean ridge system, one of Earth’s most active require a ship, which is costly and time-consuming. department Earth19 Bowl tectonic, volcanic, and biologic features. -
Final Technical Report-Cover Page
Final Technical Report Award Number G10AP00086 Sponsors Name: Seismological Society of America Conference Title: Seismological Society of America’s 2010 Annual Meeting in Portland, Oregon Conference Dates: April 21‐23, 2010 Summary of Program: This year’s SSA Annual Meeting included 282 oral presentations and 258 poster presentations distributed among 31 sessions. The meeting was attended by 557 participants from 26 countries. The meeting was preceded by the annual board meeting and committee meetings. Selected results of those meetings were shared with the membership at the annual luncheon, the first day of the meeting. Special presentations were given at the two other luncheons. The Joyner Lecture, a special lecture focusing on the boundary of seismology and engineering, was presented on Thursday night. The attached PDF contains the following: ‐ The program schedule (pages 2‐32) ‐ The meeting report including the annual luncheon minutes, the board minutes, awards presentations, and treasurer’s report (pages 33‐62) ‐ A list of registrants (Pages 63‐73) ‐ All the meeting abstracts (Pages 74‐187) SSA Annual meeting program SSA 2010 Annual Meeting Announcement Seismological Society of America Technical Sessions 21–23 April 2010 (Wednesday–Friday) Portland, Oregon IMPORTANT DATES Meeting Pre-registration Deadline 19 March 2010 Hotel Reservation Cut-Off 29 March 2010 Online Registration Cut-Off 9 April 2010 PROGRAM COMMITTEE TECHNICAL PROGRAM This year’s technical program committee is composed of co- Advances in Seismic Hazard Mapping chairs Seth Moran (USGS–Cascades Volcano Observatory) Recently much progress has been made in developing infor- and Nick Beeler (USGS–Vancouver), Ivan Wong (Seismic mative regional seismic hazard maps that incorporate local Hazards Group, Oakland CA), Ray Weldon (University of as well as regional geologic and geotechnical data. -
Earthscope Usarray Facility Final Report
EarthScope USArray Facility Final Report Award # EAR-0733069 Award Title Collaborative Research: EarthScope-Facility Operations and Maintenance (USArray) Award Term October 1, 2008 – September 30, 2013 Report Prepared on December 30, 2014 Report Prepared for National Science Foundation 4201 Wilson Boulevard Arlington, VA 22230 Report Prepared by Incorporated Research Institutions for Seismology 1200 New York Avenue, NW, Suite 400 Washington, DC 20005 Introduction The USArray component of the National Science Foundation’s EarthScope program facility consists of four major observatory components: (1) a Reference Network of permanent seismic stations; (2) a Transportable Array (TA) of ~400 seismic stations; (3) a Flexible Array (FA) pool of seismic instruments available to Principal Investigators (PIs); and (4) a Magnetotelluric (MT) observatory with permanently and temporarily deployable instruments. USArray also includes comprehensive data management and siting outreach efforts. USArray efforts during FY09–FY13 continue and expand facility activities established under the previous MREFC and O&M awards (EAR-0323309 and EAR-0323311, respectively) and continued under the “Seismological Facilities for the Advancement of Geoscience and EarthScope” award (EAR-1261681). Quarterly and annual reports submitted to the National Science Foundation throughout the award document USArray progress and accomplishments. This present report provides an overview of programmatic activities conducted under EAR- 0733069. Facility Information The Incorporated Research Institutions for Seismology (IRIS) operates USArray. Under the governance structure in place during the O&M award, USArray management received community input via the IRIS Board of Directors, the USArray Advisory Committee, and the Transportable Array and Electromagnetic Working Groups (Figure 1). The organizational structure of the USArray has been designed to leverage the experience and facilities that already exist within IRIS.